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A model for maser line profiles of late-type stars
Published online by Cambridge University Press: 04 August 2017
Abstract
The profiles of maser lines from spherically symmetric expanding shells are computed with the help of a simple model. It is shown that a beaming effect must be taken into account in order to correctly account for the OH profiles of type II OH stars.
- Type
- Circumstellar Shells and Envelopes
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 249 - 251
- Copyright
- Copyright © Reidel 1987